Q66611406

Summary

Q66611406 is a high proper-motion star^[1].

Key Facts

• Q66611406's instance of is recorded as high proper-motion star^[2].
• Q66611406's spectral class is recorded as F5V^[3].
• Q66611406's catalog code is recorded as HD 92310^[4].
• Q66611406's catalog code is recorded as FK5 4946^[5].
• Q66611406's catalog code is recorded as GSC 06637-01160^[6].
• Q66611406's catalog code is recorded as HIC 52145^[7].
• Q66611406's catalog code is recorded as HIP 52145^[8].
• Q66611406's catalog code is recorded as 2MASS J10390965-2551050^[9].
• Q66611406's catalog code is recorded as PPM 257952^[10].
• Q66611406's catalog code is recorded as SAO 179075^[11].
• Q66611406's catalog code is recorded as SRS 9819^[12].
• Q66611406's catalog code is recorded as TD1 15023^[13].
• Q66611406's catalog code is recorded as uvby98 100092310^[14].
• Q66611406's catalog code is recorded as YZ 115 8339^[15].
• Q66611406's catalog code is recorded as TYC 6637-1160-1^[16].
• Q66611406's catalog code is recorded as Gaia DR2 5469964249610379776^[17].
• Q66611406's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.63'}^[18].
• Q66611406's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.19'}^[19].
• Q66611406's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.0763'}^[20].
• Q66611406's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.329'}^[21].
• Q66611406's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.115'}^[22].
• Q66611406's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.081'}^[23].
• Q66611406's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+19.5971'}^[24].
• Q66611406's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-12.95'}^[25].
• Q66611406's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+51.0280'}^[26].

Body

Definition and Type

Q66611406's instance of is recorded as high proper-motion star^[2].